33 citations · 96 across the 6 of their papers we have counts for
6 papers
Cut-off of transverse waves through the solar transition region
Gabriel Pelouze, Tom Van Doorsselaere, Konstantinos Karampelas +2
Context. Transverse oscillations are ubiquitously observed in the solar corona, both in coronal loops and open magnetic flux tubes. Numerical simulations suggest that their dissipa…
Observational and numerical characterization of a recurrent arc-shaped front propagating along a coronal fan
M. V. Sieyra, S. Krishna Prasad, G. Stenborg +5
Recurrent, arc-shaped intensity disturbances were detected by EUV channels in an active region. The fronts were observed to propagate along a coronal loop bundle rooted in a small…
Acoustic wave properties in footpoints of coronal loops in 3D MHD simulations
Julia M. Riedl, Tom Van Doorsselaere, Fabio Reale +3
Acoustic waves excited in the photosphere and below might play an integral part in the heating of the solar chromosphere and corona. However, it is yet not fully clear how much of…
Finding the mechanism of wave energy flux damping in solar pores using numerical simulations
Julia M. Riedl, Caitlin A. Gilchrist-Millar, Tom Van Doorsselaere +2
Context. Solar magnetic pores are, due to their concentrated magnetic fields, suitable guides for magnetoacoustic waves. Recent observations have shown that propagating energy flux…
Magnetoacoustic Wave Energy Dissipation in the Atmosphere of Solar Pores
Caitlin A. Gilchrist-Millar, David B. Jess, Samuel D. T. Grant +6
The suitability of solar pores as magnetic wave guides has been a key topic of discussion in recent years. Here we present observational evidence of propagating magnetohydrodynamic…
Wave modes excited by photospheric p-modes and mode conversion in a multi-loop system
Julia M. Riedl, Tom Van Doorsselaere, Irantzu Calvo Santamaria
Context. Waves are ubiquitous in the solar corona and there are indications that they are excited by photospheric p-modes. However, it is unclear how p-modes in coronal loops are c…